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http://www.atnf.csiro.au/technology/electronics/docs/egbrkout/manual.pdf.
http://www.atnf.csiro.au/technology/electronics/docs/egbrkout/manual.pdf.
1. CSPICE Routines: GCPOOL_C
... Abstract Return the character value of a kernel variable from the kernel pool. ... Brief_I/O VARIABLE I/O DESCRIPTION -------- --- -------------------------------------------------- name I Name of the variable whose value is to be returned. start I Which component to start retrieving for name room I The largest number of values to return. lenout I The length of the output string. n O Number of values returned for name. cvals O Values associated with name. found O True if variable is in pool. ...
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Ссылки http://www.stsci.edu/~sontag/spicedocs/cspice/gcpool_c.html -- 10.2 Кб -- 17.12.2005
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2. Common Output Area and Log File
The Common Output Area (COA) on the terminal screen is the remaining top area of the terminal screen not used for the User Command Area or Task Status Area. It is a viewport on the log file. Hermes treats the log file as a ``book'' with numbered pages. ... The COA has two modes of operation: page mode and non-page mode. ... The current page number is displayed at the extreme right of the Task Status Area. ... When in non-page mode, Hermes can also scroll the COA instead of flipping pages. ...
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Ссылки http://www.atnf.csiro.au/computing/software/gipsy/hermes/COA.html -- 5.6 Кб -- 07.04.2009
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3. Outputs
Next: Tutorial Up: Fitting of Data Previous: The Fitting Process. To check any typing error or missing specification, first are displayed the options, the required precision, the maximum number of function evaluations and the method parameters. ... The reduced chi square is the . In any case, this is followed by the value of the parameters. ... If warning 2 is displayed, do again the FITting starting with the last computed value of the parameters ( nfeval < 0 in the FIT/... command). ...
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Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol1/node133.html -- 4.7 Кб -- 23.02.1996
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4. Getting the Best Performance from the API
... One of these factors is how the client application uses VDPAU; i.e. the number of surfaces allocated for buffering, order of operations, etc. ... At a bare minimum, the application must allocate one video surface for each reference frame that the stream can use (2 for MPEG or VC-1, a variable stream-dependent number for H.264) plus one surface for the picture currently being decoded. However, if this minimum number of surfaces is used, performance may be poor. ... Performance Levels . ...
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Ссылки http://www.naic.edu/~phil/hardware/nvidia/doc/driverInstall/appendix-h-section-03.html -- 7.5 Кб -- 30.10.2009
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5. RGS Related CAL Routines
Next: CAL_getBoresightMatrix Up: Routines of the Calibration Previous: List of CCF Components Contents . ... The CAL functions CAL_getBadPixelList & CAL_getBadPixelMap use the CAL state variable temperature only to check that the current operating temperature is consistent with the CCF constituent BadPix . ... Used CAL State Variables . List of CCF Components used . ... Next: CAL_getBoresightMatrix Up: Routines of the Calibration Previous: List of CCF Components Contents Michael Smith 2011-09-20 ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node252.html -- 25.8 Кб -- 20.09.2011
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6. http://xray.sai.msu.ru/~ivan/gmt/man/spectrum1d.html
spectrum1d - compute auto- [and cross- ] spectra from one [or two] timeseries. spectrum1d [ x [ y ] file ] -S segment _ size ] [ -C ] [ -D dt ] [ -N name _ stem ] [ -V ] [ -W ] [ -bi [ s ][ n ] ] [ -bo [ s ] ] spectrum1d reads X [and Y] values from the first [and second] columns on standard input [or x [ y ] file ]. ... Units same as ypower. name _ stem .npower Power spectral density of the noise output. Units same as ypower. name _ stem .gain Gain spectrum, or modulus of the transfer function. ...
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Ссылки http://xray.sai.msu.ru/~ivan/gmt/man/spectrum1d.html -- 7.0 Кб -- 19.03.1999
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7. Model realization and some results
... The perceptron structure, on the basis of which the database is built, is defined by a number of the input and output parameters and a required accuracy. ... The output perceptron data are the expansion coefficients of the scattering matrix elements in series of the generalized spherical functions. ... As the cluster structure depends on the generation conditions the expansion coefficients were averaged over 5--7 realizations of the clusters (for N . ... is the coefficient number. ...
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Ссылки http://www.astro.spbu.ru/DOP/A-PERC/PAPER2/node4.html -- 10.8 Кб -- 19.11.2010
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8. The Apache TPF Port
Configuration Files | ... Options | ... This version of Apache includes changes allowing it to run on IBM's EBCDIC-based TPF (Transaction Processing Facility) operating system. ... It is passed to Apache through the ZINET XPARM field since ZINET is the only way to start the server on TPF. A third group of options apply to both the informational displays (ZFILE) and running the server (ZINET XPARM): -d, -D and -f. The rest of Apache's options are either not applicable or are not supported on TPF. ...
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Ссылки http://neptun.sai.msu.su/manual/readme-tpf.html -- 22.1 Кб -- 05.11.2004
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9. http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIFringeTrackerSW.DesignDocuments/StepData.txt
... I've included typical values in some cases: int num_gd_trials; /** Number of trial group delays */ int num_bas ; /** Number of baselines measured by FT (up to 9) */ int num_channels = 5; /** Number of spectral channels used for fringe tracking */ int num_output; /** Total number of combiner outputs in use */ int num_win = 5; /** Number of windows (subframes) per camera : TODO : not needed? */ Monitor Data ===== /** * Pixel data at a modulator position from all cameras. ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIFringeTrackerSW.DesignDocuments/StepData.txt -- 4.6 Кб -- 17.10.2011
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10. refreshVCAL
... This tool creates a set of virtual calibrations (vcalibs). It is thought to be used in case an existing set of virtual calibrations got lost, is required, and would be difficult or time-consuming to be created in the standard way (by subsequent creation of ABs). ... The user specifies a starting date, from where the tool counts a number of dates backwards (either by reading N_VCAL_LIST in config.createAB, or by specifying a command line parameter). ... for a specified, non-standard number of days. ...
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Ссылки http://www.eso.org/~qc/dfos/refreshVCAL.html -- 6.3 Кб -- 19.12.2006
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11. Gadget Box PPS Level Converter and CHU Modem
... It includes level converters and a optional radio modem designed to decode the radio timecode signals transmitted by the Canadian time and frequency station CHU. A complete set of schematics, PCB artwork, drill templates is in the pub/ntp/gadget.tar.Z file on ftp.udel.edu. ... One of these converts a TTL positive edge into a fixed- width pulse at EIA levels and is for use with a timecode receiver or oscillator including a TTL PPS output. ... See the schematic diagram gadget.s01 for reference. ...
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Ссылки http://www.sai.msu.su/~er/xntp/gadget.html -- 6.3 Кб -- 21.12.2007
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12. Recursion
A completely new possibility of Fortran 90 is recursion. Note that it requires that you give a new property RESULT for the output variable in the function declaration. ... Here follows two examples, first recursive calculation of the factorial, then recursive calculations of the Fibonacci-numbers. ... The listings of the routines follow, the output variables are called FAC_RESULT and FIBO_RESULT , respectively. ... Not only functions but also subroutines can be recursive. ...
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Ссылки http://star.arm.ac.uk/f77to90/c9.html -- 4.8 Кб -- 17.02.1996
[ Сохраненная копия ] Ссылки http://crydee.sai.msu.ru/f90/c9.html -- 4.8 Кб -- 17.02.1996
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13. A Spectroscopy Exposure Time Calculator for IRAF
... Up: Iraf Packages . ... IRAF Group, NOAO 1 , PO Box 26732, Tucson, AZ 85726 . This paper describes a new IRAF spectroscopy exposure time calculator. ... SPTIME takes an input source spectrum, either a reference blackbody, power law, or a user spectrum, a background ``sky'', observing parameters such as exposure time, central wavelength, seeing, airmass, and moon phase, instrument parameters such as aperture sizes and detector binning, a description of the spectrograph, and desired output. ...
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Ссылки http://www.adass.org/adass/proceedings/adass99/P1-45/ -- 10.7 Кб -- 12.10.2000
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14. HSTPOLSIM (V1.00) --- April99 --- HSTPOLSIM (V1.00)
hstpolsim -- Produce simulated polarization input data frames for HST instruments . ... inint = "" [name] . ... Name of the HST instrument for which simulated polarization images are to be produced. ... Name of the instrument specific polarizing filter for simulated images (ignored for SPECIAL instrument). filtname = "" [name] . Name of the instrument specific colour filter for simulated images. ... The header parameter FILTER provides the filter name and POLANG the polarizer angle. ...
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Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/impol/hstpolsim.help.html -- 11.0 Кб -- 06.06.2006
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15. Two-Temperature Raymond Model
Next: Limiting Energy Channels Input Up: *fit* - Fit Data Previous: Raymond Model . The model is a two-temperature Raymond thermal spectrum, low temperature range is 0.55 to 0.65 keV, high temperature range is 1 to 2 keV, element abundance table is cosmic, abundance of heavy elements (atomic number >2 ) is 50% of the value in the table. Note that 0.7 = log(5.0), specifies that the second component normalization will be 5 times the normalization of the first component. ...
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node149.html -- 4.0 Кб -- 01.10.2012
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16. Siding Spring Survey
T he Siding Spring Survey (SSS) is a Near-Earth Object search program that utilises the 0.5-m Uppsala Schmidt Telescope at Siding Spring Observatory, N.S.W., Australia. ... The mission of the Siding Spring Survey is to contribute to the inventory of near-earth objects (NEOs), or more specifically, the potentially hazardous asteroids (PHAs) and comets (PHOs) that may pose a threat of impact and thus harm to civilization. ... Based on the CSS Mission page . ... Siding Spring Survey Main Page . ...
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Ссылки http://www.mso.anu.edu.au/~rmn/ -- 11.4 Кб -- 23.12.2011
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17. Getting Started in Actor Prolog. Component-Oriented Programming.
The idea of component-oriented programming is that in the course of implementation of various software projects a programmer (or a programmers team) accumulates a library of reused software fragments that are used in different projects. ... To solve such problems there are some special syntax means in Actor Prolog that support component-oriented programming. ... A package in Actor Prolog is a set of classes linked by implication. ... Actor Prolog supports visual component-oriented programming. ...
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Ссылки http://www.cplire.ru/Lab144/start/e_comp.html -- 18.6 Кб -- 24.09.2007
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18. Electronics
The HAWAII detector is an array of HgCdTe photodiodes whose junction capacity collects a charge proportional to the number of photons that they receive. ... The array detector is read by an electronic system based on the controller developed by the CCD Working Group of TNG, modified to speed up the read-out time, and on a fast 16 bit conversion board (2 Mb/s). ... The signal read on each pixels is buffered by electronics located on the same board that hosts the detector. ...
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Ссылки http://www.arcetri.astro.it/irlab/instr/nics/generale/elettr.html -- 5.3 Кб -- 28.07.2005
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19. SCL Spectrum Commands
... spectrum . ... sfit . ... Briefly, these refer to the type of spectrum to be computed, the method of calculation of the source function, the number of anges if specific intensities are to be computed, the choice of continuous opacity subroutine library, the broadening data for HeI lines and the approximation ito be used for untabulated diffuse HeI lines. ... Refer to the SPECTRUM documentation for more information. spc_nsource <nsource> : Switch for method used to compute source function (def: 3) . ...
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Ссылки http://star.arm.ac.uk/~csj/software_store/guide/scl_spc.html -- 5.8 Кб -- 30.08.2007
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20. Writing programs that use comedi and comedilib
Comedi Documentation . ... Right to the source: #include <stdio.h> /* for printf() */ #include <comedilib.h> int subdev = 0; /* change this to your input subdevice */ int chan = 0; /* change this to your channel */ int range = 0; /* more on this later */ int aref = AREF_GROUND; /* more on this later */ int main(int argc,char *argv[]) { comedi_t *it; lsampl_t data; it=comedi_open("/dev/comedi0"); comedi_data_read(it,subdev,chan,range,aref,&data); printf("%d\n",data); return 0; } . ...
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Ссылки http://mavr.sao.ru/hq/sts/linux/comedi/doc/x94.html -- 8.9 Кб -- 28.12.2007
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